Collections

VizieR astronomical catalogues

  J/A+A/493/L17 - VLTI observations of V4334 Sgr (Chesneau+, 2009)

We present high spatial resolution observations in the mid-infrared of the Sakurai's object (V4334 Sgr) obtained with the Very Large Telescope Interferometer (VLTI) of ESO's Paranal Observatory and MIDI, the MID-infrared Interferometric recombiner. MIDI combines the light of two telescopes and provi…

0 observation logs, 7 granules in 2 OIFITS files.
From
to

  J/A+A/536/A55 - Milli-arcsecond imaging of SS Lep (Blind+, 2011)

The observations made use of the VLTI instruments AMBER and PIONIER. The data are reduced. AMBER ones were obtained from archive data of ESO (program IDs: 082.D-0019(A); 082.D-0019(B); 082.D-0019(D); 082.D-0062(A); 082.D-0019(E); 083.D-0028(A)). PIONIER data were obtained during the commissioning of…

0 observation logs, 15 granules in 8 OIFITS files.
From
to

  J/A+A/544/A91 - {epsilon} Aur visibility measurements (Mourard+, 2012)

VEGA/CHARA interferometric observations in differential mode are provided in the attached files, according to the OIFITS format.

0 observation logs, 63 granules in 63 OIFITS files.
From
to

  J/A+A/545/A130 - Interferometry of {alpha} Eri (Domiciano de Souza+, 2012)

We used the AMBER focal instrument at ESO-VLTI in its high spectral resolution mode to record interferometric data on the fast rotator Achernar. Differential phases centered on the hydrogen Br{gamma} line (K band) were obtained during four almost consecutive nights with a continuous Earth-rotation s…

0 observation logs, 28 granules in 28 OIFITS files.
From
to

  J/A+A/558/A149 - VLTI/MIDI AGN Large Program observations (Burtscher+, 2013)

All interferometric observations were carried out with MIDI, the MID-infrared interferometric Instrument at the European Southern Observatory's (ESO's) Very Large Telescope Interferometer (VLTI) on Cerro Paranal, Chile. The MIDI AGN Large Program (ESO program number 184.B-0832) consisted of 13.1 ni…

0 observation logs, 144 granules in 23 OIFITS files.
From
to

  J/A+A/558/A24 - The VLTI/MIDI survey of Massive YSOs (Boley+, 2013)

We provide the complete set of reduced, spectrally-resolved MIDI visibilities and differential phases for the 20 objects observed as part of the survey presented in the above publication. These interferometric data are provided in FITS format, and, more specifically, conform to the OIFITS standard (…

0 observation logs, 148 granules in 20 OIFITS files.
From
to

  J/A+A/559/A111 - 89 Her interferometric study (Hillen+, 2013)

89 Herculis was observed with the AMBER instrument on the VLTI using the Auxiliary Telescopes (ATs) in 2007, 2008, and 2012, all in the low-spectral-resolution (R=30) mode covering the H and K bands with detector integration times (DITs) of 25 and 50ms and without the use of the fringe tracker FINIT…

0 observation logs, 28 granules in 14 OIFITS files.
From
to

  J/A+A/565/A71 - NGC1068 MIDI/VLTI observations (Lopez-Gonzaga+, 2014)

The low spatial frequency interferometric observations of NGC 1068 were carried out using the 1.8m Auxiliary Telescopes (AT's) together with the MID-infrared interferometric Instrument (MIDI) at the European Southern Observatory's (ESO's) Very Large Telescope Interferometer (VLTI) on Cerro Paranal, …

0 observation logs, 6 granules in 1 OIFITS files.
From
to

  J/A+A/586/A35 - TZ For OIFITS files (Gallenne+, 2016)

We collected high-resolution echelle spectra from the instruments Euler/CORALIE and 3.6m/HARPS located at La Silla Observatory (Chile). We used the Very Large Telescope Interferometer (VLTI) with the four-telescope combiner PIONIER to measure the squared visibilities and the closure phases. Our ob…

0 observation logs, 11 granules in 11 OIFITS files.
From
to

  J/A+A/593/A45 - VEGA/CHARA interferometric observations of Cepheids I. A resolved structure around the prototype classical Cepheid delta Cep in the visible spectral range

Context. The B-W method is used to determine the distance of Cepheids and consists in combining the angular size variations of the star, as derived from infrared surface-brightness relations or interferometry, with its linear size variation, as deduced from visible spectroscopy using the projection …

0 observation logs, 205 granules in 179 OIFITS files.
From
to

  J/A+A/597/A137 - HD 123999 and Alpha Cen A and B OIFITS files (Kervella+, 2017)

The files contain all the PIONIER calibrated interferometric data obtained on Alpha Centauri A and B, as well as on the dimensional calibrator HD 123999. The data files follow the OIFITS standard of optical interferometry as defined by Pauls et al. (2005PASP..117.1255P).

0 observation logs, 13 granules in 13 OIFITS files.
From
to

  J/A+A/602/A78 - NGC1068 interferometric mid-IR measurements (Lopez-Gonzaga+, 2017)

Single-aperture mid-infrared images and spectra were taken with the VLT spectrometer and imager for the mid-infrared (VISIR). Interferometric measurements were obtained with the instrument MIDI at the ESO's VLTI facility. Observations with intermediate AT baselines were requested and observed duri…

0 observation logs, 3 granules in 1 OIFITS files.
From
to

Other collections

  VEGA Import - VEGA observation logs

This collection gathers VEGA observation logs.

3743 observation logs, 0 granules in 0 OIFITS files.
From
to

  CLIMB/CLASSIC import - CLIMB/CLASSIC observation logs

This collection gathers CLIMB/CLASSIC observation logs from CHARA.

32346 observation logs, 0 granules in 0 OIFITS files.
From
to

  IOTA - IOTA L2 data

0 observation logs, 285 granules in 105 OIFITS files.
From
to

  V854 Cen - The R CrB star V854 Cen

This dataset is the one that allowed O. Chesneau to discover a hot dusty shell around the R Corona Borealis star V854 Cen. Visibilities and closure phases vary continuously from the H to the K bands, giving evidence of a hot-dust component in the system.

0 observation logs, 24 granules in 24 OIFITS files.
From
to

  V838 Mon - AMBER and MIDI observations of V838 Mon

These are the data used in the paper of O. Chesneau to resolve the central star of the system and find it has shrunk by la large factor in a decade. The MIDI data also show a disc-like structure around the star that may be the result of the 2002 outburst.

0 observation logs, 16 granules in 16 OIFITS files.
From
to

  T Pyx - T Pyx AMBER observations

These two oifits files correspond to the Chesneau paper from 2011 on the T Pyxidis nova observations. These data allowed us to detect a face-on bipolar fireball at the nova explosion time. These data were processed again with a more recent version of amdlib, as the original published data could not …

0 observation logs, 2 granules in 2 OIFITS files.
From
to

  PIONIER - PIONIER L2 data

0 observation logs, 6386 granules in 6373 OIFITS files.
From
to

  Gomes+2016 collection - to be completed - Study data - to be completed (Gomes+, 2016)

Associated simulated material is not indexed by the OiDB database, but is archived and online on the associated JMMC server. This is a set of OIFITS data files generated with OI-SIM – a Yorick package with functions useful to simulate interferometric observations – and that were used to study …

0 observation logs, 0 granules in 0 OIFITS files.
From
to

  HAeBeLP - Calibrated data of the Herbig Large Program PIONIER/VLTI

All the oifits used in: Structure of Herbig AeBe disks at the milliarcsecond scale. A statistical survey in the H band using PIONIER-VLTI B. Lazareff, J.-P. Berger, J. Kluska, J.-B. Le Bouquin, M. Benisty, F. Malbet, C. Koen, C. Pinte, W.-F. Thi, and 20 more co-authors. DOI: http://dx.doi.org/10.1…

0 observation logs, 278 granules in 235 OIFITS files.
From
to

  Gamma Vel - AMBER observations of Gamma Velorum

A follow-up observing program on Gamma Vel.

0 observation logs, 43 granules in 43 OIFITS files.
From
to